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RATAN-600 Observation Schedule from 1 July to 31 December, 2019 Executive Secretary: request@sao.ru |
Russian version |
North Sector | South+Flat | South Sector | West Sector | |
---|---|---|---|---|
J U L Y |
Feed-cabin 1 (01-31): Radio properties of the Narrow-Line Seyfert 1 Galaxies, (01-31): Radio variability of the Galactic X-ray binaries with relativistic jets, (01-31): Radio properties of the blazars on the long time scales, |
Feed-cabin 3 (01-31): The Sun five-azimuth observations 3. (01-31): Repairs, (01-31): Antenna measurements, |
(01-31): Repairs, (01-31): Antenna measurements, |
Feed-cabin 5 (01-31): Test observations (SAO RAS). |
A U G U S T |
Feed-cabin 1 (01-31): Radio variability of the Galactic X-ray binaries with relativistic jets, (01-10): Study of the long-term variability of the extragalactic radio sources in the declination range from 11 up to 18 degrees, (11-31): Radio properties of the distant quasars, (11-31): Radio properties of the Narrow-Line Seyfert 1 Galaxies, |
Feed-cabin 3 (01-31): The Sun five-azimuth observations 3. (01-31): Repairs, (01-31): Antenna measurements, |
(01-31): Repairs, (01-31): Antenna measurements, |
Feed-cabin 5 (01-31): Test observations (SAO RAS). |
S E P T E M B E R |
Feed-cabin 1 (01-30): The AGN study with the RATAN-600 and VLBI 2, (01-30): Radio variability of the Galactic X-ray binaries with relativistic jets1, |
Feed-cabin 3 (01-30): The Sun five-azimuth observations 3. (01-30): Repairs, (01-30): Antenna measurements, |
(01-30): Repairs, (01-30): Antenna measurements, |
Feed-cabin 5 (01-30): Test observations (SAO RAS). |
O C T O B E R |
Feed-cabin 1 (01-01): The AGN study with the RATAN-600 and VLBI 2, (01-01): Radio variability of the Galactic X-ray binaries with relativistic jets1, (02-04): Reserve time (SAO RAS) (05-17): Technical support, (18-31): Adjustment, antenna measurements, |
Feed-cabin 3 (01-31): The Sun five-azimuth observations 3. (01-31): Repairs, (01-31): Antenna measurements, |
(01-31): Repairs, (01-31): Antenna measurements, |
Feed-cabin 5 (01-31): Test observations (SAO RAS). |
N O V E M B E R |
Feed-cabin 1 (01-02): Reserve time (03-30): Radio variability of the Galactic X-ray binaries with relativistic jets, (03-12): Study of the long-term variability of the extragalactic radio sources in the declination range from 11 up to 18 degrees, (13-30): Radio properties of the blazars on the long time scales, (13-30): Radio properties of the Narrow-Line Seyfert 1 Galaxies, |
(01-15): Repairs, (01-15): Adjustment, antenna measurements, Feed-cabin 3 (01-30): The Sun five-azimuth observations 3. (16-20): Reserve time (SAO RAS) Feed-cabin 2 (21-30): Radio properties of the blazars on the long time scales, (21-30): Radio properties of the Narrow-Line Seyfert 1 Galaxies, (21-30): Radio variability of the Galactic X-ray binaries with relativistic jets, |
(01-15): Technical support, (01-15): Adjustment, antenna measurements, (16-20): Reserve time Feed-cabin 2 (21-30): Radio variability of the Galactic X-ray binaries with relativistic jets, |
Feed-cabin 5 (01-30): Test observations (SAO RAS). |
D E C E M B E R |
Feed-cabin 1 (01-31): Radio variability of the Galactic X-ray binaries with relativistic jets, (01-20): Radio properties of the blazars on the long time scales, (01-20): Radio properties of the Narrow-Line Seyfert 1 Galaxies, (21-31): Study of the long-term variability of the extragalactic radio sources in the declination range from 11 up to 18 degrees, |
Feed-cabin 2 (01-31): Radio variability of the Galactic X-ray binaries with relativistic jets, (01-31): Radio properties of the blazars on the long time scales, (01-31): Radio properties of the Narrow-Line Seyfert 1 Galaxies, Feed-cabin 3 (01-31): The Sun multi-azimuth observations 3. Testing of the antenna system (South+Flat) in the tracking mode. |
Feed-cabin 2 (01-31): Radio variability of the Galactic X-ray binaries with relativistic jets, |
Feed-cabin 5 (01-31): Test observations (SAO RAS). |
1 - During a trigger.
2 - ICRANet Italy; University of Oxford UK; INAF-IAPS Italy; SAO USA; Finnish Center for Astronomy with ESO FINCA.
3 - Structure and evolution of solar active regions (Alissandrakis C., University of Ioannina, Greece); Magnetosphere of the active region in a wide frequency range (Bogod V.M., SAO RAS); Study of the solar floccules in the CaIIK line and in the microwave range with GAS GAO and RATAN-600 (Tlatov A.G., GAO RAS); Investigation of ultra-weak solar activity (Lesovoy S.V., ISTP SB RAS); Study of the chromosphere and the transition region of sunspots with ALMA interferometer and RATAN-600 (M. Lukicheva, NJIT, USA).
4 - NRAO, USA; Shanghai Astronomical Observatory, China; Max-Planck-Insitut für Radioastronomie, Germany; Joint Institute for VLBI in Europe; IRA INAF, Italy; Netherlands Institute for Radio Astronomy, Netherlands.
Feed-cabin 1 - secondary mirror with complex equipment
of the continuous spectrum of 1.28-21.7 GHz.
Feed-cabin 2 - secondary mirror with complex equipment
of the continuous spectrum of 2.25-21.7 GHz (ERIDAN).
Feed-cabin 3 - secondary mirror with solar
spectral-polarization complex.